Binary interactions and cluster dynamics boost PISN rates by up to 3x versus single stars, enabling constraints on stellar-wind mass loss and galaxy metallicity distributions.
and Kalirai, Jason S
4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
years
2026 4representative citing papers
MESA grid models of Procyon A and B give a system age of 2.23 Gyr, white dwarf cooling age of 1.20 Gyr, and map the progenitor to the 1.9-2.6 solar mass range with higher core overshoot than standard.
Tentative evidence for a super-Jupiter at 15-100 AU or brown dwarf at 20-170 AU in 51 Pegasi from RV curvature, but the signal is likely driven by Lick/Hamilton instrument drift.
NODSV is a new public catalog of ~1400 symbiotic binaries with classifications into confirmed, candidate, and misidentified categories plus a statistical overview of their properties.
citing papers explorer
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Analysis of DQZ White Dwarf Evolution through Procyon
MESA grid models of Procyon A and B give a system age of 2.23 Gyr, white dwarf cooling age of 1.20 Gyr, and map the progenitor to the 1.9-2.6 solar mass range with higher core overshoot than standard.
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New Online Database of Symbiotic Variables: Catalog and Statistical Overview of Symbiotic Binaries
NODSV is a new public catalog of ~1400 symbiotic binaries with classifications into confirmed, candidate, and misidentified categories plus a statistical overview of their properties.